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Helioseismology has taught us a great deal about the stratification andkinematics of the solar interior, sufficient for us to embark upon dynamicalstudies more detailed than have been possible before. The most sophisticatedstudies to date have been the very impressive numerical simulations of theconvection zone, from which, especially in recent years, a great deal has beenlearnt. Those simulations, and the seismological evidence with which they arebeing confronted, are reviewed elsewhere in this volume. Our understanding ofthe global dynamics of the radiative interior of the Sun is in a much moreprimitive state. Nevertheless, some progress has been made, and seismologicalinference has provided us with evidence of more to come. Some of that Isummarize here, mentioning in passing hints that are pointing the way to thefuture.

Some glimpses from helioseismology at the dynamics of the deep solar interior